J/A+A/565/A7    Transit observations of the super-Earth GJ1214b (Caceres+, 2014)

Ground-based transit observations of the super-Earth GJ1214b. Caceres C., Kabath P., Hoyer S., Ivanov V.D., Rojo P., Girard J.H., Miller-Ricci Kempton E., Fortney J.J., Minniti D. <Astron. Astrophys. 565, A7 (2014)> =2014A&A...565A...7C 2014A&A...565A...7C
ADC_Keywords: Stars, double and multiple ; Planets; Photometry Keywords: planetary systems - techniques: photometric - techniques: spectroscopic - planets and satellites: atmospheres - stars: individual: GJ 1214 Abstract: GJ 1214b is one of the few known transiting super-Earth-sized exoplanets with a measured mass and radius. It orbits an M-dwarf, only 14.55pc away, making it a favorable candidate for follow-up studies. However, the composition of GJ 1214b's mysterious atmosphere has yet to be fully unveiled. Our goal is to distinguish between the various proposed atmospheric models to explain the properties of GJ 1214b: hydrogen-rich or hydrogen-He mix, or a heavy molecular weight atmosphere with reflecting high clouds, as latest studies have suggested. Wavelength-dependent planetary radii measurements from the transit depths in the optical/NIR are the best tool to investigate the atmosphere of GJ 1214b. We present here (i) photometric transit observations with a narrow-band filter centered on 2.14-microns and a broad-band I-Bessel filter centered on 0.8665-microns, and (ii) transmission spectroscopy in the H and K atmospheric windows that cover three transits. The obtained photometric and spectrophotometric time series were analyzed with MCMC simulations to measure the planetary radii as a function of wavelength. We determined radii ratios of 0.1173 for I-Bessel and 0.11735 at 2.14-microns. Our measurements indicate a flat transmission spectrum, in agreement with last atmospheric models that favor featureless spectra with clouds and high molecular weight compositions. Description: Files contain data points from the obtained light curves of the transiting planet GJ 1214b we obtained with the SOI (in the I-Bessel filter) and OSIRIS (with a narrow-band filter centered on 2.14um) instruments at the SOAR telescope. They include the BJD of observation, the measured flux, and the photometric error estimation. Objects: -------------------------------------------------- RA (2000) DE Designation(s) -------------------------------------------------- 17 15 18.94 +04 57 49.7 GJ 1214b = GJ 1214b -------------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file phot1.dat 30 1466 Photometry obtained with SOI (with I-Bessel filter) phot2.dat 30 1030 Photometry obtained with OSIRIS (with a 2.14um narrow-band filter) -------------------------------------------------------------------------------- See also: J/A+A/549/A10 : Transits of GJ 1214 (Harpsoe+, 2013) Byte-by-byte Description of file: phot1.dat phot2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 16 F16.8 d BJD Time of observation (TDB) 18- 23 F6.4 --- Flux Normalized flux 25- 30 F6.4 --- e_Flux Error in normalized flux -------------------------------------------------------------------------------- Acknowledgements: Claudio Caceres, ccaceres(at)dfa.uv.cl
(End) C. Caceres [Univ. de Valparaiso, Chile], P. Vannier [CDS] 13-Mar-2014
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line